Spaceship Escape speed understanding

AI Thread Summary
The discussion revolves around calculating the final speed of a spaceship when it is far from Earth after being launched with an initial speed. Participants explore the relationship between kinetic energy and gravitational potential energy, emphasizing that the spaceship drifts without propulsion after launch. The initial kinetic energy is expressed as (1/2)mv^2, while the gravitational potential energy is represented as -G(Mm/R). The key point is to equate the total mechanical energy at launch to the kinetic energy at a significant distance from Earth, where potential energy approaches zero. The conversation highlights the importance of simplifying equations and understanding the concepts of energy conservation in this context.
Patdon10
Messages
85
Reaction score
0

Homework Statement


A spaceship is launched from the Earth's surface with a speed v. The radius of the Earth is R. What will its speed be when it is very far from the Earth? (Use any variable or symbol stated above along with the following as necessary: G for the gravitational constant, m for the mass of the spaceship, and M for the mass of the Earth.)

What is V_f?


2. The attempt at a solution

I'm really not sure what my teacher is looking for. I tried sqroot(2GM/R) to no avail. Any ideas?

I also know vf = vi + at. What could I substitute in for the acceleration?
 
Physics news on Phys.org
Patdon10 said:
I also know vf = vi + at. What could I substitute in for the acceleration?
The vf - vi = at formula only works for uniform acceleration. But that doesn't apply here because the acceleration changes throughout the trip.

And by the way, I'm pretty sure you're supposed to assume that the spaceship was launched into space as if launched from a catapult. In other words, once it gets away from the Earth's surface, it drifts naturally without using any significant thrust or propulsion. Assume the ship uses up all of its propulsion/fuel/etc, when launching, immediately after which the spaceship has mass m and speed v.

Here are some questions to ask yourself.
  • What is the initial kinetic energy of the spaceship?
  • What is the gravitational potential of Earth (with respect to infinity)?
  • Knowing Earth's gravitational potential, what is the difference in gravitational potential energy between a spaceship of mass m on the surface of the Earth and infinity?
  • So after reaching an infinite distance from Earth (well, let's just say "a long way from Earth"), how much kinetic energy is left over?
 
The equation I'm getting is total energy = (1/2)mv^2 - G*(mM/R+h)

How could I solve for v final from having the total energy? h = infinity
 
Patdon10 said:
The equation I'm getting is total energy = (1/2)mv^2 - G*(mM/R)
'Looks good :approve: but just make sure you note that the v in the above equation is the initial speed, vi.
K.E.final = ½mvi2 - G(Mm/R)​
How could I solve for v final from having the total energy?
Ummm, :rolleyes: I'm sure you already know this,
K.E.final = ½mvf2
 
well, yeah. I know that final kinetic energy is equal to that. However, why is it kinetic energy? Isn't it total Mechanical energy?...

You know what, you're right. Isn't it only kinetic energy because the potential energy is 0 (it's very far away)?
 
I tried
Untitled1-1.png
Still telling me it's the wrong answer : /
 
Patdon10 said:
I tried
Untitled1-1.png



Still telling me it's the wrong answer : /
I don't see anything wrong with your answer. But the program might be expecting you to simplify a little more maybe. You could multiply the 2/m through the other terms, getting rid of the variable m in the process.
 
Alright. I'll give it a try. Thanks a lot for the speedy responses.
 
Back
Top